Initial performance of the radio occultation experiment in the Venus orbiter mission Akatsuki
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- Material Type
- 記事
- Author/Editor
- Takeshi ImamuraHiroki AndoSilvia Tellmann
- Publication, Distribution, etc.
- Publication Date
- 2017-10-03
- Publication Date (W3CDTF)
- 2017-10-03
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 69(137)
- Volume
- 69(137)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-017-0722-3
- Persistent ID (NDL)
- info:ndljp/pid/11002663
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2017-12-14T17:18:17+09:00
- Date Captured (W3CDTF)
- 2017-12-12
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/10319651
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- コレクション : 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- DOI
- 10.1186/s40623-017-0722-3
- Access Restrictions
- インターネット公開
- Rights (production)
- © The Author(s) 2017.This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
- Related Material
- Initial performance of the radio occultation experiment in the Venus orbiter mission Akatsuki
- Related Material (URI)
- Is Referenced By
- Planetary-scale streak structure reproduced in a Venus atmospheric simulationStationary Features at the Cloud Top of Venus Observed by Ultraviolet Imager Onboard AkatsukiQuasi‐Periodic Variation of the Lower Equatorial Cloud Induced by Atmospheric Waves on VenusPeriodic Variation of Mesoscale Ultraviolet Contrast at the Cloud Top of VenusX-band scintillations in Venus radio occultations observed by AkatsukiProbing solar wind velocity from simultaneous superior solar conjunction radio science experiments of BepiColombo and Akatsuki missionsShort vertical wavelength gravity waves in the Martian polar lower atmosphere observed by reanalysis of Mars Global Surveyor radio occultation dataLunar meter-wave telescope (TSUKUYOMI) as one of Japanese lunar plansFine Vertical Structures at the Cloud Heights of Venus Revealed by Radio Holographic Analysis of Venus Express and Akatsuki Radio Occultation DataHorizontal structures of bow-shaped mountain wave trains seen in thermal infrared images of venusian clouds taken by Akatsuki LIRGravity Wave Packets in the Venusian Atmosphere Observed by Radio Occultation Experiments: Comparison With Saturation TheoryA Recharge Oscillator Model for Interannual Variability in Venus’ CloudsDynamical Effect on Static Stability of the Venus Atmosphere Simulated Using a General Circulation Model: A Comparison With Radio Occultation MeasurementsCharacteristic Features of <i>V</i><sub>0</sub> Layer in the Venus Ionosphere as Observed by the Akatsuki Orbiter: Evidence for Its Presence During the Local Noon and Post‐Sunset ConditionsObservation of the Solar Corona Using Radio Scintillation with the Akatsuki Spacecraft: Difference Between Fast and Slow WindOne-dimensional Microphysics Model of Venusian Clouds from 40 to 100 km: Impact of the Middle-atmosphere Eddy Transport and SOIR Temperature Profile on the Cloud StructureDensity fluctuation in the solar corona and solar wind: A comparative analysis of radio-occultation observations and magnetohydrodynamic simulationLocal Time Dependence of the Thermal Structure in the Venusian Equatorial Upper Atmosphere: Comparison of Akatsuki Radio Occultation Measurements and GCM ResultsVenusian Ionosphere During Deep Solar Minima: Some New Insights Using Akatsuki Radio Science ExperimentEvaluation of new radio occultation observations among small satellites at Venus by data assimilationThe nightside cloud-top circulation of the atmosphere of VenusCorrelation of Venusian Mesoscale Cloud Morphology Between Images Acquired at Various WavelengthsGravity Wave Modulations at the Lower Altitudes of Venus IonosphereThermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultation惑星大気の衛星間電波掩蔽観測のための最適軌道に関する研究Venus Climate Orbiter Akatsuki RS Doppler Profiles PDS3 datasetVenus Climate Orbiter Akatsuki RS Bending Angle and Temperature/Pressure Profiles PDS3 datasetEvaluation of a method to retrieve temperature and wind velocity profiles of the Venusian nightside mesosphere from mid-infrared CO2 absorption line observed by heterodyne spectroscopyUltraviolet imager on Venus orbiter Akatsuki and its initial resultsSpecial issue “Akatsuki at Venus : the first year of scientific operation”Influence of the cloud-level neutral layer on the vertical propagation of topographically generated gravity waves on Venus
- References
- Radio occultation measurement of the electron density near the lunar surface using a subsatellite on the SELENE missionSmall-scale temperature fluctuations seen by the VeRa Radio Science Experiment on Venus ExpressMeasurements of thermal structure and thermal contrasts in the atmosphere of Venus and related dynamical observations: Results From the four Pioneer Venus ProbesThe structure of Venus’ middle atmosphere and ionosphereDensities and temperatures in the Venus mesosphere and lower thermosphere retrieved from SOIR on board Venus Express: Carbon dioxide measurements at the Venus terminatorZonal Winds in the Middle Atmosphere of Venus from Pioneer Venus Radio Occultation DataThe atmosphere of mars analyzed by integral inversion of the Mariner IV occultation dataA Numerical Microphysical Model of the Condensational Venus CloudVenus cloud formation in the meridional circulationInternal structure of a coronal mass ejection revealed by Akatsuki radio occultation observationsVertical Wavenumber Spectra of Gravity Waves in the Venus Atmosphere Obtained from Venus Express Radio Occultation Data: Evidence for SaturationH2O-H2SO4 System in Venus' Clouds and OCS, CO, and H2SO4 Profiles in Venus' TroposphereVertical structure of the atmosphere of Venus from Pioneer Venus Orbiter radio occultationsGreenhouse models of Venus' High surface temperature, as constrained by Pioneer Venus measurementsMicrowave absorptivity by sulfuric acid in the Venus atmosphere: First results from the Venus Express Radio Science experiment VeRaModels of the structure of the atmosphere of Venus from the surface to 100 kilometers altitudeQuantification of middle and lower cloud variability and mesoscale dynamics from Venus Express/VIRTIS observations at 1.74μmMagellan Radio Occultation Measurements of Atmospheric Waves on VenusObservable effects of convection and gravity waves on the Venus condensational cloudThe Refractive Indices and Dielectric Constants of Air and its Principal Constituents at 24,000 Mc/sRadio Occultation Studies of the Venus Atmosphere with the Magellan SpacecraftRADIAL DISTRIBUTION OF COMPRESSIVE WAVES IN THE SOLAR CORONA REVEALED BY<i>AKATSUKI</i>RADIO OCCULTATION OBSERVATIONSRadio occultation measurements of turbulence in the Venus atmosphere by Pioneer VenusDynamical properties of the Venus mesosphere from the radio-occultation experiment VeRa onboard Venus ExpressRadio Scintillations in Venus's Atmosphere: Application of a Theory of Gravity Wave GenerationRadio science investigations by VeRa onboard the Venus Express spacecraftThe Microwave Absorption and Abundance of Sulfuric Acid Vapor in the Venus Atmosphere Based on New Laboratory MeasurementsStatistical and computational uncertainties in atmospheric profiles from radio occultation: Mariner 10 at VenusThe radio occultation method for the study of planetary atmospheresThe Neutral Atmosphere of Venus as Studied with the Mariner V Radio Occultation ExperimentsRadio propagation experiments in the outer solar system with VoyagerModeling the effects of shear on the evolution of the holes in the condensational clouds of VenusMicrophysics of Venusian Clouds in Rising Tropical AirOUTFLOW STRUCTURE OF THE QUIET SUN CORONA PROBED BY SPACECRAFT RADIO SCINTILLATIONS IN STRONG SCATTERINGInverse insolation dependence of Venus’ cloud-level convectionStudying the Lunar Ionosphere with SELENE Radio Science ExperimentThe thermal structure of the Venus atmosphere: Intercomparison of Venus Express and ground based observations of vertical temperature and density profilesSolar cycle effects on the structure of the electron density profiles in the dayside ionosphere of VenusStructure of the Venus neutral atmosphere as observed by the Radio Science experiment VeRa on Venus ExpressFlight Model Development of PLANET-C Telecommunication SubsystemVenus Climate Orbiter Akatsuki RS Doppler Profiles PDS3 datasetVenus Climate Orbiter Akatsuki RS Bending Angle and Temperature/Pressure Profiles PDS3 datasetOverview of Venus orbiter, AkatsukiRadio occultation experiment of the Venus atmosphere and ionosphere with the Venus orbiter AkatsukiAKATSUKI returns to Venus
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 学術機関リポジトリデータベース雑誌記事索引データベースCrossrefCiNii Articles科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベースJapan Link CenterJapan Link CenterJapan Link CenterJapan Link Center学術機関リポジトリデータベースCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossref
- Bibliographic ID (NDL)
- 11002663
- NAID
- 120006486821